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Volumn 395, Issue 1, 2002, Pages

An explanation for the curious mass loss history of massive stars: From OB stars, through Luminous Blue Variables to Wolf-Rayet stars

Author keywords

Stars: evolution; Stars: Luminous Blue Variables Stars: OB; Stars: mass loss; Stars: Wolf Rayet

Indexed keywords

LUMINESCENCE; RADIATION EFFECTS; SPACE RESEARCH; WIND;

EID: 0036851075     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021381     Document Type: Article
Times cited : (36)

References (21)
  • 7
    • 0003050340 scopus 로고    scopus 로고
    • Luminous Blue Variables, Massive stars in transition, ed. A. Nota, & H.J.G.L.M. Lamers
    • Lamers, H.J.G.L.M. 1997, in Luminous Blue Variables, Massive stars in transition, ed. A. Nota, & H.J.G.L.M. Lamers, ASP Conf. Ser., 120, 76.
    • (1997) ASP Conf. Ser. , vol.120 , pp. 76
    • Lamers, H.J.G.L.M.1
  • 9
    • 0001916114 scopus 로고    scopus 로고
    • ed. A. Nota, & H.J.G.L.M. Lamers
    • Leitherer, C. 1997, in ASP Conf. Ser. 120, ed. A. Nota, & H.J.G.L.M. Lamers, 58.
    • (1997) ASP Conf. Ser. , vol.120 , pp. 58
    • Leitherer, C.1
  • 18
    • 0001641699 scopus 로고    scopus 로고
    • Schmutz, W. 1997, A & A, 321, 268.
    • (1997) A & A , vol.321 , pp. 268
    • Schmutz, W.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.